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The 67P/Churyumov–Gerasimenko observation campaign in support of the Rosetta mission

Snodgrass, C., A'Hearn, M. F., Aceituno, F., Afanasiev, V., Bagnulo, S., Bauer, J., Bergond, G., Besse, S., Biver, N., Bodewits, D., and others. (2017) The 67P/Churyumov–Gerasimenko observation campaign in support of the Rosetta mission. Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, 375 (2097). ISSN 1364-503X. (doi:10.1098/rsta.2016.0249)

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Abstract

We present a summary of the campaign of remote observations that supported the European Space Agency's Rosetta mission. Telescopes across the globe (and in space) followed comet 67P/Churyumov–Gerasimenko from before Rosetta's arrival until nearly the end of the mission in September 2016. These provided essential data for mission planning, large-scale context information for the coma and tails beyond the spacecraft and a way to directly compare 67P with other comets. The observations revealed 67P to be a relatively ‘well-behaved’ comet, typical of Jupiter family comets and with activity patterns that repeat from orbit to orbit. Comparison between this large collection of telescopic observations and the in situ results from Rosetta will allow us to better understand comet coma chemistry and structure. This work is just beginning as the mission ends—in this paper, we present a summary of the ground-based observations and early results, and point to many questions that will be addressed in future studies.

Item Type: Article
DOI/Identification number: 10.1098/rsta.2016.0249
Uncontrolled keywords: Orbits; Space flight, 67p/churyumov-gerasimenko; Context information; European Space Agency; Ground-based observations; Jupiter-family comets; Observations; Remote observation; Rosetta, Interplanetary flight
Subjects: Q Science > QC Physics
Divisions: Faculties > Sciences > School of Physical Sciences > Centre for Astrophysics and Planetary Sciences
Depositing User: Stephen Lowry
Date Deposited: 11 Jul 2017 11:38 UTC
Last Modified: 12 Jul 2019 10:05 UTC
Resource URI: https://kar.kent.ac.uk/id/eprint/62250 (The current URI for this page, for reference purposes)
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